The SPHEREx Sky Simulator: Science Data Modeling for the First All-sky Near-infrared Spectral Survey

Abstract We describe the SPHEREx Sky Simulator (henceforth the Simulator), a software tool designed to model science data for NASA’s SPHEREx mission that will carry out a series of all-sky spectrophotometric surveys at ∼6″ spatial resolution in 102 spectral channels spanning 0.75–5 μ m. The Simulator software implements models for astrophysical emission, instrument characteristics, and survey strategy to generate realistic infrared sky scenes as they will be observed by SPHEREx. The simulated data include a variety of realistic noise and systematic effects that are estimated using up-to-date astrophysical measurements and information from prelaunch instrument characterization campaigns. Through the preflight mission phases, the Simulator has been critical in predicting the impact of various effects on SPHEREx science performance and has played an important role in guiding the development of the SPHEREx data analysis pipeline. In this paper, we describe the Simulator architecture, preflight instrument, and sky models, and summarize high-level predictions from the Simulator, including a prelaunch prediction for the 5 σ point source sensitivity of SPHEREx, which we estimate to be m AB 18.5–19 from 0.75 to 3.8 μ m and m AB 16.6–18 from 3.8 to 5 μ m, with the sensitivity limited by the zodiacal light background at all wavelengths. In the future, on-orbit data will be used to improve the Simulator, which will form the basis of a variety of forward-modeling tools that will be used to model myriad instrumental and astrophysical processes to characterize their systematic effects on our final data products and analyses.

Authors

Publication Details

Journal
The Astrophysical Journal Supplement Series
Published
2025-10-27
DOI
https://doi.org/10.3847/1538-4365/ae04cc
Citations
5
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
5.77
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article

The SPHEREx Sky Simulator: Science Data Modeling for the First All-sky Near-infrared Spectral Survey

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The Astrophysical Journal Supplement Series
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article

The SPHEREx Sky Simulator: Science Data Modeling for the First All-sky Near-infrared Spectral Survey

Yi-Kuan Chiang, Sean Bryan, Volker Tolls, S. Everett, Tzu‐Ching Chang, C. D. Dowell, Tatiana Goldina, Yujin Yang, Richard M. Feder, Phillip Korngut, B. P. Crill, Woong-Seob Jeong, Zhaoyu Huai, M. Zemcov, Rachel Akeson, Teresa Symons, H. Hui, A. Cukierman, Daniel Masters, Candice Fazar, Asantha Cooray, Yun-Ting Cheng, J. Kang, M. L. N. Ashby, M. W. Werner, J. J. Bock, Andreas L. Faisst, Yoonsoo P. Bach, Jae‐Joon Lee, Jeonghyun Pyo, Olivier Doré, Chi H. Nguyen, Jean Choppin de Janvry
article en
5 citations

Abstract

Abstract We describe the SPHEREx Sky Simulator (henceforth the Simulator), a software tool designed to model science data for NASA’s SPHEREx mission that will carry out a series of all-sky spectrophotometric surveys at ∼6″ spatial resolution in 102 spectral channels spanning 0.75–5 μ m. The Simulator software implements models for astrophysical emission, instrument characteristics, and survey strategy to generate realistic infrared sky scenes as they will be observed by SPHEREx. The simulated data include a variety of realistic noise and systematic effects that are estimated using up-to-date astrophysical measurements and information from prelaunch instrument characterization campaigns. Through the preflight mission phases, the Simulator has been critical in predicting the impact of various effects on SPHEREx science performance and has played an important role in guiding the development of the SPHEREx data analysis pipeline. In this paper, we describe the Simulator architecture, preflight instrument, and sky models, and summarize high-level predictions from the Simulator, including a prelaunch prediction for the 5 σ point source sensitivity of SPHEREx, which we estimate to be m AB 18.5–19 from 0.75 to 3.8 μ m and m AB 16.6–18 from 3.8 to 5 μ m, with the sensitivity limited by the zodiacal light background at all wavelengths. In the future, on-orbit data will be used to improve the Simulator, which will form the basis of a variety of forward-modeling tools that will be used to model myriad instrumental and astrophysical processes to characterize their systematic effects on our final data products and analyses.

The Astrophysical Journal Supplement SeriesVol. 281(1)
Openalex Percentile: Top 4%
Galaxies: Formation, Evolution, Phenomena
5.77
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